Planck’s dusty GEMS: The brightest gravitationally lensed galaxies discovered with the Planck all-sky survey

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Volume 581 (September 2015)

A&A, 581 (2015) A105

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Table 1

Mid-IR to millimetre photometry.

Source	Survey	RA	Dec	z _source	z _fg,sdss	S ₂₂	S ₂₅₀	S ₃₅₀	S ₅₀₀	S ₈₅₀	S ₂₀₀₀

		(J2000)	(J2000)			[mJy]	[mJy]	[mJy]	[mJy]	[mJy]	[mJy]

PLCK_G045.1+61.1	OT2	15:02:36.04	+29:20:51	3.4	0.56^a^,^b	<5.4	161 ± 5	328 ± 6	397 ± 6	130 ± 13	13 ± 2
PLCK_G080.2+49.8	OT2	15:44:32.40	+50:23:46	2.6	0.5	<5.4	220 ± 9	340 ± 6	314 ± 6	87 ± 5	7 ± 2
PLCK_G092.5+42.9	PCCS	16:09:17.76	+60:45:21	3.3	0.5	<5.4	765 ± 7	865 ± 8	696 ± 7	191 ± 16	8.4 ± 0.6
PLCK_G102.1+53.6	OT2	14:29:17.98	+59:21:09	2.9	0.74^a	8.1 ± 0.7	327 ± 4	410 ± 5	339 ± 5	...	5.5 ± 0.7
PLCK_G113.7+61.0	PCCS	13:23:02.88	+55:36:01	2.4	0.3	6.0 ± 0.7	672 ± 7	603 ± 6	373 ± 5	108 ± 10	4±1
PLCK_G138.6+62.0	PCCS	12:02:07.68	+53:34:40	2.4	0.4	6.2 ± 0.8	619 ± 6	664 ± 8	474 ± 6	123 ± 14	7±1
PLCK_G145.2+50.9	PCCS	10:53:22.56	+60:51:49	3.6	...	<5.4	453 ± 5	719 ± 7	781 ± 8	360 ± 23	38±4
PLCK_G165.7+67.0	PCCS	11:27:14.60	+42:28:25	2.2	0.34^a,b	10.4 ± 0.9	867 ± 8	753 ± 6	472 ± 5	90 ± 9	8±1
PLCK_G200.6+46.1	OT2	09:32:23.67	+27:25:00	3.0	0.6	<5.4	209 ± 4	294 ± 4	273 ± 5	110 ± 10	7±2
PLCK_G231.3+72.2	OT2	11:39:21.60	+20:24:53	2.9	0.1	<5.4	299 ± 4	401 ± 5	341 ± 6	111 ± 12	9 ± 1
PLCK_G244.8+54.9	PCCS	10:53:53.04	+05:56:21	3.0	0.13	<5.4	1050 ± 10	1054 ± 10	777 ± 7	198 ± 11	19 ± 2

HLS-J0918^c		09:18:28.6	+51:42:23	5.2			85 ± 8	168 ± 8	203 ± 9	125 ± 8	15 ± 7
HATLAS-J1146^d		11:46:37.9	−00:11:32	3.3			323 ± 24	378 ± 28	298 ± 24	93 ± 12	38 ± 6

Notes. The columns are: source name; indication of whether the sources come from the PCCS or our own high-z selection (OT2, see Sect. 2); RA and Dec coordinates; redshift of the high-z source; SDSS redshift of the intervening foreground source; WISE 22-μm flux density; Herschel-SPIRE 250-μm flux density; Herschel-SPIRE 350-μm flux density; Herschel-SPIRE 500-μm flux density; JCMT/SCUBA-2 850-μm flux density; and IRAM 30-m/GISMO 2-mm flux density.

^(a)

Spectroscopic redshift of intervening foreground source from the SDSS.

^(b)

Multiple foreground sources at a common spectroscopic redshift near the line of sight.

^(c)

This source has been found with the Herschel Lensing Survey and has previously been discussed by Combes et al. (2012) and Rawle et al. (2014). The last column lists the 1.2-mm flux density measured with MAMBO on the IRAM 30-m telescope.

^(d)

This source from the ERCSC (Planck Collaboration VII 2011) falls serendipitously into the HATLAS field and has been previously discussed by Fu et al. (2012). The last column lists the 1.2-mm flux density measured with MAMBO on the IRAM 30-m telescope.

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